Tidal dissipation due to the elliptical instability and turbulent viscosity in convection zones in rotating giant planets and stars (2023)
Attributed to:
The DiRAC 2.5x Facility
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2306.17622
Publication URI: https://arxiv.org/abs/2306.17622
Type: Other